A SAURON study of M32: measuring the intrinsic flattening and the central black hole mass

We present dynamical models of the nearby compact elliptical galaxy M32, using high-quality kinematic measurements, obtained with the integral-field spectrograph SAURON mounted on the William Herschel Telescope on La Palma. We also include STIS data obtained previously by Joseph et al. We find a best-fitting black hole mass of M-. = (2.5 +/- 0.5) x 10(6) M. and a stellar I-band mass-to-light ratio of (1.85 +/- 0.15) M./L.. For the first time, we are also able to constrain the inclination along which M32 is observed to 70degrees +/- 5degrees. Assuming that M32 is indeed axisymmetric, the averaged observed flattening of 0.73 then corresponds to an intrinsic flattening of 0.68 +/- 0.03. These tight constraints are mainly caused by the use of integral-field data. We show this quantitatively by comparing with models that are constrained by multiple slits only. We show the phase-space distribution and intrinsic velocity structure of the best-fitting model and investigate the effect of regularization on the orbit distribution.